activity
20062025
most citedGeometrical constraints on the origin of timing signals from black holes

190 citations · 2.6k across the 115 of their papers we have counts for

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11 papers · 1 filter

astro-ph.HE2022★ 19 cited

Timing analysis of the 2022 outburst of the accreting millisecond X-ray pulsar SAX J1808.43658: hints of an orbital shrinking

Giulia Illiano, Alessandro Papitto, Andrea Sanna +19

We present a pulse timing analysis of NICER observations of the accreting millisecond X-ray pulsar SAX J1808.43658 during the outburst that started on 2022 August 19. Similar to…

astro-ph.HE2022★ 14 cited

The AstroSat observation of accreting millisecond X-ray pulsar SAX J1808.4-3658 during its 2019 outburst

Rahul Sharma, Andrea Sanna, Aru Beri

We report on the analysis of the AstroSat dataset of the accreting millisecond X-ray pulsar SAX J1808.4-3658, obtained during its 2019 outburst. We found coherent pulsations at $\s…

astro-ph.HE2022★ 7 cited

Spectral analysis of the AMXP IGR J17591-2342 during its 2018 outburst

A. Manca, A. F. Gambino, A. Sanna +9

The Accreting Millisecond X-ray Pulsar IGR J17591-2342 is a LMXB system that went in outburst on August 2018 and it was monitored by the NICER observatory and partially by other fa…

gr-qc2022

Semiclassical spacetimes at super-Planckian scales from delocalized sources

Ali Akil, Mariano Cadoni, Leonardo Modesto +2

We derive the gravitational field and the spacetime metric generated by sources in quantum superposition of different locations. We start by working in a Newtonian approximation, i…

astro-ph.HE2022★ 9 cited

The thermonuclear X-ray bursts of 4U 1730-22

Peter Bult, Giulio C. Mancuso, Tod E. Strohmayer +11

We present observations of the historic transient 4U 1730-22 as observed with the Neutron Star Interior Composition Explorer (NICER). After remaining in quiescence since its 1972 d…

astro-ph.HE2022★ 20 cited

MAXI J1957+032: a new accreting millisecond X-ray pulsar in an ultra-compact binary

A. Sanna, P. Bult, M. NG +12

The detection of coherent X-ray pulsations at ~314 Hz (3.2 ms) classifies MAXI J1957+032 as a fast-rotating, accreting neutron star. We present the temporal and spectral analysis p…